Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
44.5419 -8.9579 0.0161 53.0564 169.5545 11.4549532 11.887 TRIG_00922968
Foreground time interval of the image:
-51.896 12.005 (delta_t = 63.901 [sec])
Background time interval of the image:
-153.795 -51.896 (delta_t = 101.899 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -51.896 sec. to 7.240 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.56418 ( -0.205265 0.221602 )
Norm@50keV : 1.05722E-02 ( -0.00163808 0.00161571 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.98 using 59 PHA bins.
# Reduced chi-squared = 0.9295 for 57 degrees of freedom
# Null hypothesis probability = 6.265477e-01
Photon flux (15-150 keV) in 59.14 sec: 2.16162 ( -0.21713 0.21736 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.36796e-06 ( -7.16233e-07 7.29149e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -51.896 sec. to 7.240 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36963 ( -1.57487 0.642839 )
Epeak [keV] : 18.8978 ( )
Norm@50keV : 5.94836E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.25 using 59 PHA bins.
# Reduced chi-squared = 0.8794 for 56 degrees of freedom
# Null hypothesis probability = 7.264320e-01
Photon flux (15-150 keV) in 59.14 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -51.896 sec. to 7.240 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.25630 (-0.717116 0.802749)
R^2/D10^2 : 3.45194 (-1.25671 1.97236)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.83 using 59 PHA bins.
# Reduced chi-squared = 0.9971 for 57 degrees of freedom
# Null hypothesis probability = 4.813487e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.790e-06 3.007e-07
25- 50 2.625e-06 3.548e-07
50-150 4.946e-07 1.739e-07
15-150 4.910e-06 6.659e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 30.6061 (-6.24772 8.4265)
Norm : 16.9165 (-3.45113 4.55221)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.22 using 59 PHA bins.
# Reduced chi-squared = 0.8634 for 57 degrees of freedom
# Null hypothesis probability = 7.586482e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.057e-06 2.916e-07
25- 50 2.376e-06 2.883e-07
50-150 1.336e-06 4.447e-07
15-150 5.769e-06 7.289e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.06675 (-1.51051 1.10112)
R1^2/D10^2 : 6.35827 (-2.95272 10.0259)
kT2 [keV] : 19.4565 (-14.8994 38.4446)
R2^2/D10^2 : 2.34384E-02 (-0.0228419 0.407888)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.93 using 59 PHA bins.
# Reduced chi-squared = 0.8715 for 55 degrees of freedom
# Null hypothesis probability = 7.391200e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.970e-06 6.012e-07
25- 50 2.408e-06 7.759e-07
50-150 1.580e-06 9.712e-07
15-150 5.958e-06 1.997e-06
Peak spectrum fit
Power-law model
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.23166 ( -0.301917 0.360041 )
Norm@50keV : 5.50036E-02 ( -0.0149091 0.0147579 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.28 using 59 PHA bins.
# Reduced chi-squared = 1.022 for 57 degrees of freedom
# Null hypothesis probability = 4.281806e-01
Photon flux (15-150 keV) in 1 sec: 17.9964 ( -2.7245 2.7275 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.42027e-07 ( -1.16926e-07 1.17659e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 80.0000 ( )
Norm@50keV : 0.106818 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 131.66 using 59 PHA bins.
# Reduced chi-squared = 2.3510 for 56 degrees of freedom
# Null hypothesis probability = 4.936829e-08
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -0.012 sec. to 0.988 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.10907 (-1.02002 1.11056)
R^2/D10^2 : 58.7752 (-31.43 78.9823)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.20 using 59 PHA bins.
# Reduced chi-squared = 1.091 for 57 degrees of freedom
# Null hypothesis probability = 2.962433e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.990e-07 8.625e-08
25- 50 3.100e-07 8.560e-08
50-150 3.054e-08 1.749e-08
15-150 6.395e-07 1.629e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.5022 (-4.79757 6.08733)
Norm : 223.452 (-69.8494 116.011)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.50 using 59 PHA bins.
# Reduced chi-squared = 0.9737 for 57 degrees of freedom
# Null hypothesis probability = 5.314081e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.391e-07 7.130e-08
25- 50 2.912e-07 6.100e-08
50-150 8.357e-08 4.233e-08
15-150 7.139e-07 1.335e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.15792 (-1.6598 1.99121)
R1^2/D10^2 : 905.732 (-806.165 154401)
kT2 [keV] : 8.73259 (-2.28048 5.30746)
R2^2/D10^2 : 8.22301 (-7.74501 32.4566)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.91 using 59 PHA bins.
# Reduced chi-squared = 0.9984 for 55 degrees of freedom
# Null hypothesis probability = 4.780387e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.513e-07 1.926e-07
25- 50 2.835e-07 1.527e-07
50-150 8.468e-08 5.640e-08
15-150 7.195e-07 3.564e-07
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.56418 ( -0.205265 0.221602 )
Norm@50keV : 1.05722E-02 ( -0.00163808 0.00161571 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.98 using 59 PHA bins.
# Reduced chi-squared = 0.9295 for 57 degrees of freedom
# Null hypothesis probability = 6.265477e-01
Photon flux (15-150 keV) in 59.14 sec: 2.16129 ( -0.217083 0.217319 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.3663e-06 ( -7.15961e-07 7.29261e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36835 ( -1.57406 0.628711 )
Epeak [keV] : 18.9147 ( -16.3372 9.89541 )
Norm@50keV : 5.95967E-02 ( -0.0598652 0.583037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.25 using 59 PHA bins.
# Reduced chi-squared = 0.8794 for 56 degrees of freedom
# Null hypothesis probability = 7.264317e-01
Photon flux (15-150 keV) in 59.14 sec: 2.07730 ( -0.22876 0.22906 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.77152e-06 ( -7.83014e-07 8.70139e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.12e-06
S(50-100 keV) = 1.44e-06
T90 vs. Hardness ratio plot
T90 = 56.8959999084473 sec.
Hardness ratio (energy fluence ratio) = 0.679245
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.00377
Count Ratio (50-100 keV) / (15-25 keV) = 0.336588
Mask shadow pattern
IMX = -1.307727448355517E+00, IMY = -2.410857632435768E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-153.795410 -51.896000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
342.9171 -29.1791 2.4 39.3 81.9 4.0342 4.8 ------ UNKNOWN
338.3553 -30.9460 2.4 39.9 75.2 4.5459 4.8 ------ UNKNOWN
27.1653 -14.1734 2.4 44.9 148.5 4.4040 4.8 ------ UNKNOWN
303.6921 -50.3429 2.5 42.9 25.7 1.8258 4.6 ------ UNKNOWN
16.5381 -48.7423 2.4 10.4 124.0 1.1339 4.9 ------ UNKNOWN
65.4878 -32.7404 2.4 39.5 -151.7 1.6657 4.8 ------ UNKNOWN
89.7463 -72.3481 2.8 29.3 -75.6 1.2521 4.1 ------ UNKNOWN
86.3455 -61.0966 2.7 31.5 -97.7 1.4761 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-51.896000 7.240000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
44.5426 -8.9549 1.1 53.1 169.6 11.3343 11.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
86.004600 662.984000
720.904000 963.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
23.7252 28.2696 3.0 42.3 158.7 14.8415 3.8 ------ UNKNOWN
53.9167 29.3317 3.5 39.4 -160.7 7.8039 3.3 ------ UNKNOWN
66.2059 -12.7564 2.3 21.6 -71.7 8.9953 4.9 ------ UNKNOWN
74.6902 -9.1561 2.6 29.8 -80.9 9.6354 4.4 ------ UNKNOWN
Plot creation:
Wed Oct 9 17:57:49 EDT 2019